3D continuum radiative transfer in complex dust configurations around stellar objects and active galactic nuclei. I. Computational methods and capabilities

Astronomy and Astrophysics

Volumn 401, Issue 2, 2003, Pages 405-418

  Steinacker, J ^a   Henning, Th ^b   Bacmann, A ^c   Semenov, D ^a  

^a FRIEDRICH SCHILLER UNIVERSITY JENA   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Accretion, accretion disks; ISM: dust extinction; Methods: numerical; Radiative transfer

Indexed keywords

ALGORITHMS; DUST; GALAXIES; ULTRAVIOLET RADIATION;

STELLAR OBJECTS;

ASTROPHYSICS;

EID: 0037388356     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021853     Document Type: Article

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